activity
20032026
most citedGaia-ESO Survey: The analysis of high-resolution UVES spectra of FGK-type stars

227 citations · 4.3k across the 103 of their papers we have counts for

collaborators

103 papers

astro-ph.SR2026

Open Clusters as Laboratories for Cool Star Evolution: Highlights from the Cool Stars 23 Splinter Session

Deepak Chahal, Beatrice Caccherano, Edward Gillen +16

Open clusters remain among the most powerful laboratories for calibrating how fundamental stellar properties such as rotation, magnetic activity, surface chemistry, and internal st…

astro-ph.IM2026

SHARPing accretion and outflows in young stellar objects in star forming regions of the outer Galaxy and beyond

Juan Manuel Alcala', Alessio Caratti o Garatti, Linda Podio +5

As part of the science book of SHARP, we present here the science case of star-disk interaction of low-mass (\Mstar2\Msun) young stellar objects (YSOs), in low-metallicity (Z…

astro-ph.EP2026

The PLATO field selection process III. Selection of the Prime Sample for the LOPS2 field

V. Nascimbeni, G. Piotto, V. Granata +30

The PLanetary Transits and Oscillations of stars (PLATO) mission will begin its four-year nominal mission in early 2027 by monitoring its Long-duration Observation Phase field at S…

astro-ph.EP2026★ 1 cited

The PLATO Input Catalogue of targets (tPIC) for the first Long Pointing Field

M. Montalto, G. Piotto, P. M. Marrese +31

The ESA PLAnetary Transits and Oscillations of stars (PLATO) mission is designed to detect terrestrial planets in the habitable zones of solar-type stars. Owing to telemetry constr…

astro-ph.SR2025

Using a neural network approach and starspots dependent models to predict effective temperatures and ages of young stars

Marco Tarantino, Loredana Prisinzano, Nicoletta D Angelo +2

This study presents a statistical approach to accurately predict the effective temperatures of pre-main sequence stars, which are necessary for determining stellar ages using the i…

astro-ph.IM2025

The Dynamics of the Milky Way: Unveiling the 6D Skeleton of Star Formation in the 2040s

Loredana Prisinzano, Germano G. Sacco, Francesco Damiani +5

The Milky Way (MW) is our unique laboratory to test star formation theories at the level of individual stars, serving as the Rosetta Stone to interpret extragalactic observations.…